Preprints
https://doi.org/10.5194/egusphere-2026-3834
https://doi.org/10.5194/egusphere-2026-3834
08 Jul 2026
 | 08 Jul 2026
Status: this preprint is open for discussion and under review for Climate of the Past (CP).

Dynamical Mechanism behind the Southern Hemisphere Westerly Intensification during the Last Glacial Maximum: A Linkage between Sea-ice and Polar Front Jet

Hyeong-Gyu Kim, Joowan Kim, Sang-Yoon Jun, Seong-Joong Kim, and Damwon So

Abstract. The Southern Hemisphere westerlies (SHW) play a pivotal role in modulating the global carbon cycle and climate feedback. However, their behavior during the Last Glacial Maximum (LGM) is debated owing to discrepancies between paleoclimate models and proxy records. While tropical upper-tropospheric cooling and Antarctic surface cooling exert opposing influences on the SHW, the detailed dynamical mechanisms through which Antarctic sea-ice expansion modulates large-scale atmospheric circulation are poorly understood. In this study, we investigated the dynamical mechanisms of austral winter SHW change under altered orbital and surface conditions with a series of climate model simulations. By conducting sensitivity experiments with varying Antarctic sea-ice concentrations, we isolated the thermodynamic effect of sea ice from the tropical cooling signal. Our results demonstrate that sea-ice-induced surface cooling drives the poleward intensification of the SHW through two distinct mechanisms. First, strong surface cooling steepens the meridional temperature gradient near the sea-ice edge, thereby directly maintaining the SHW intensity through thermal wind balance. Second, the enhanced baroclinicity amplifies eddy heat fluxes and storm track activity. The resulting increase in storm track activity drives a downward transfer of upper-tropospheric westerly momentum, reinforcing the surface westerlies. Through these mechanisms, the sea-ice-driven cooling outweighed the opposing equatorward influence of tropical cooling. This study provides a dynamical framework for understanding how sea-ice thermodynamic forcing drives large-scale circulation changes in the context of LGM climate conditions.

Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims made in the text, published maps, institutional affiliations, or any other geographical representation in this paper. While Copernicus Publications makes every effort to include appropriate place names, the final responsibility lies with the authors. Views expressed in the text are those of the authors and do not necessarily reflect the views of the publisher.
Share
Hyeong-Gyu Kim, Joowan Kim, Sang-Yoon Jun, Seong-Joong Kim, and Damwon So

Status: open (until 02 Sep 2026)

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
Hyeong-Gyu Kim, Joowan Kim, Sang-Yoon Jun, Seong-Joong Kim, and Damwon So
Hyeong-Gyu Kim, Joowan Kim, Sang-Yoon Jun, Seong-Joong Kim, and Damwon So
Metrics will be available soon.
Latest update: 08 Jul 2026
Download
Short summary
The westerly winds over the Southern Ocean influence ocean currents and the global carbon cycle, yet how they behaved during the last ice age remains uncertain. Using a global climate model, we tested how the expansion of Antarctic sea ice affected these winds. The sea ice cooled the surface, strengthening the winds and shifting them toward Antarctica, outweighing the opposite pull from a colder tropics. Our results show Antarctic sea ice is a key driver of these winds in past climates.
Share